CERN Accelerating science

002838147 001__ 2838147
002838147 003__ SzGeCERN
002838147 005__ 20221027180819.0
002838147 0247_ $$2DOI$$a10.22323/1.314.0616
002838147 0248_ $$aoai:cds.cern.ch:2838147$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
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002838147 035__ $$9Inspire$$a1664827
002838147 041__ $$aeng
002838147 100__ $$aGraziani, Maura$$uPerugia U.
002838147 245__ $$aPrecise and Systematic Long-duration Study of Solar Modulation on Elementary Particles and Nuclei with AMS-02 on the Space Station
002838147 260__ $$bSISSA$$c2017
002838147 300__ $$a4 p
002838147 520__ $$9SISSA$$aWe present the precise monthly time variation of the $e^{+}$, $e^{-}$, $p$ and $He$ fluxes by the Alpha Magnetic Spectrometer on the International Space Station. The data were collected during the ascending phase of solar cycle $\#$24 through its maximum and toward its minimum. This covers one half solar cycle. For the first time, the time evolution of cosmic rays of opposite charges and different mass and charge are simultaneously measured during the reversal of the Sun's magnetic field polarity. These measurements are crucial for solar modulation modelling during periods of high-level solar activity. They also provide constraints for modelling astrophysical backgrounds for dark matter searches.
002838147 540__ $$aCC BY-NC-ND 4.0$$bSISSA$$uhttps://creativecommons.org/licenses/by-nc-nd/4.0/
002838147 542__ $$dthe author(s)$$g2018
002838147 595__ $$aFor annual report
002838147 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002838147 690C_ $$aARTICLE
002838147 690C_ $$aCERN
002838147 693__ $$aAMS
002838147 710__ $$gAMS Collaboration
002838147 773__ $$01664112$$c616$$pPoS$$vEPS-HEP2017$$wC17-07-05$$y2017
002838147 8564_ $$82402358$$s340303$$uhttp://cds.cern.ch/record/2838147/files/PoS(EPS-HEP2017)616.pdf$$yFulltext
002838147 960__ $$a13
002838147 962__ $$b2234151$$k616$$nvenice20170705
002838147 980__ $$aARTICLE
002838147 980__ $$aConferencePaper